Table 4: The flux of LBQS 2212-1759 as a function of wavelength, from the near-IR to the EUV. The values in the optical and UV have been obtained by averaging fluxes from individual OM exposures. All fluxes have been corrected for foreground galactic reddening.
Instrument ${\rm\lambda_{obs}}$ ${\rm\Delta\lambda_{obs}}$ ${\rm\lambda_{rest}}$ ${\rm\Delta\lambda_{rest}}$ Flux
  (Å) ( ${\rm 10^{-16}~erg~cm^{-2}~s^{-1}~\AA^{-1}}$)
2MASS K 21 590 2620 6711 814 $0.945\pm0.047$
2MASS H 16 620 2510 5166 780 $1.006\pm0.071$
2MASS J 12 350 1620 3839 504 $0.987\pm0.082$
OM-V 5430 710 1688 221 $2.957\pm0.040$
OM-B 4500 980 1399 305 $4.673\pm0.018$
OM-U 3440 780 1069 242 $4.478\pm0.026$
OM-UVW1 2910 710 905 221 $4.186\pm0.013$
OM-UVM2 2310 460 718 143 $3.447\pm0.082$
OM-UVW2 2120 460 659 143 $2.868\pm0.379$


Source LaTeX | All tables | In the text